Inspired by the Kerr/CFT proposal for some magnetized black holes [1]}, [2]}, [3]}, we extend the conjecture to the case of MRNTN case. To proceed, first we need to obtain the corresponding near horizon and accompanying vector solution in an extremal MRNTN geometry. It turns out that resulting near horizon metric and the vector field solution are compatible with the general form that is used in the asymptotic symmetry group method [4]}. Therefore, the general formula for the central charge and Frolov-Thorne temperature achieved in [4]} can apply. In section , we recover the extremal entropy for a MRNTN black hole by using Cardy formula as prescribed by Kerr/CFT correspondence [6]}, [4]}, [8]}.
